Publication: Revised event rates for extreme and extremely large mass-ratio inspirals
Revised event rates for extreme and extremely large mass-ratio inspirals
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Vázquez-Aceves, V., Zwick, L., Bortolas, E., Capelo, P. R., Amaro Seoane, P., Mayer, L., & Chen, X. (2022). Revised event rates for extreme and extremely large mass-ratio inspirals. Monthly Notices of the Royal Astronomical Society, 510(2), 2379–2390. https://doi.org/10.1093/mnras/stab3485
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One of the main targets of the Laser Interferometer Space Antenna (LISA) is the detection of extreme mass-ratio inspirals (EMRIs) and extremely large mass-ratio inspirals (X-MRIs). Their orbits are expected to be highly eccentric and relativistic when entering the LISA band. Under these circumstances, the inspiral time-scale given by Peters’ formula loses precision and the shift of the last-stable orbit (LSO) caused by the massive black hole spin could influence the event rates estimate. We re-derive EMRIs and X-MRIs event rates by im
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- Vázquez-Aceves, Verónica
- Zwick, Lorenz
- Bortolas, Elisa
- Capelo, Pedro R
- Amaro Seoane, Pau
- Mayer, Lucio
- Chen, Xian
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Vázquez-Aceves, V., Zwick, L., Bortolas, E., Capelo, P. R., Amaro Seoane, P., Mayer, L., & Chen, X. (2022). Revised event rates for extreme and extremely large mass-ratio inspirals. Monthly Notices of the Royal Astronomical Society, 510(2), 2379–2390. https://doi.org/10.1093/mnras/stab3485
